eccentric planets
eccentric planets
eccentric planets
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No metallicity effect for low mass <strong>planets</strong><br />
Mayor et al. 2011<br />
•HARPS high precision sample: [Fe/H] for giant gaseous <strong>planets</strong> (black), for <strong>planets</strong> less<br />
massive than 30 ME (red), and for the global combined sample stars (blue).<br />
•No metallicity effect for low mass <strong>planets</strong>.<br />
•Even absence of low mass <strong>planets</strong> at high [Fe/H]?<br />
•Natural outcome in the core accretion formation model.<br />
?<br />
?<br />
Mayor et al. 2011
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